| |
|
|
|
|
|
|
|
|
1. |
Record Nr. |
UNINA9910254576303321 |
|
|
Autore |
Stadnik Yevgeny V |
|
|
Titolo |
Manifestations of Dark Matter and Variations of the Fundamental Constants in Atoms and Astrophysical Phenomena / / by Yevgeny V. Stadnik |
|
|
|
|
|
|
|
Pubbl/distr/stampa |
|
|
Cham : , : Springer International Publishing : , : Imprint : Springer, , 2017 |
|
|
|
|
|
|
|
|
|
ISBN |
|
|
|
|
|
|
Edizione |
[1st ed. 2017.] |
|
|
|
|
|
Descrizione fisica |
|
1 online resource (XXI, 88 p. 22 illus., 18 illus. in color.) |
|
|
|
|
|
|
Collana |
|
Springer Theses, Recognizing Outstanding Ph.D. Research, , 2190-5053 |
|
|
|
|
|
|
|
|
Disciplina |
|
|
|
|
|
|
Soggetti |
|
Gravitation |
Astronomy |
Astrophysics |
Atoms |
Physics |
Particles (Nuclear physics) |
Quantum field theory |
Classical and Quantum Gravitation, Relativity Theory |
Astronomy, Astrophysics and Cosmology |
Atomic, Molecular, Optical and Plasma Physics |
Elementary Particles, Quantum Field Theory |
|
|
|
|
|
|
|
|
Lingua di pubblicazione |
|
|
|
|
|
|
Formato |
Materiale a stampa |
|
|
|
|
|
Livello bibliografico |
Monografia |
|
|
|
|
|
Nota di bibliografia |
|
Includes bibliographical references. |
|
|
|
|
|
|
Nota di contenuto |
|
Introduction -- New Methods of Axion Dark Matter Detection -- New Methods of Scalar Dark Matter Detection -- New Spectroscopy Methods to Search for Anomalous Fifth-Forces -- Concluding Remarks. |
|
|
|
|
|
|
|
|
Sommario/riassunto |
|
This thesis explores the possibility of searching for new effects of dark matter that are linear in g, an approach that offers enormous advantages over conventional schemes, since the interaction constant g is very small, g<<1. Further, the thesis employs an investigation of linear effects to derive new limits on certain interactions of dark matter with ordinary matter that improve on previous limits by up to 15 orders of magnitude. The first-ever limits on several other interactions are |
|
|
|
|
|
|
|
|
|
|
also derived. Astrophysical observations indicate that there is five times more dark matter—an ‘invisible’ form of matter, the identity and properties of which still remain shrouded in mystery—in the Universe than the ordinary ‘visible’ matter that makes up stars, planets, dust and interstellar gases. Conventional schemes for the direct detection of dark matter involve processes (such as collisions with, absorption by or inter-conversion with ordinary matter) that are either quartic (g4) or quadratic (g2) in an underlying interaction constant g. |
|
|
|
|
|
| |